The Impact of Void-finding Algorithms on Galaxy Classification

Journal Article · 20 December 2024 · The Astrophysical Journal

DOI: https://doi.org/10.3847/1538-4357/ad9585 · OSTI ID:2483618

Zaidouni, Fatima ; Veyrat, Dahlia ; Douglass, Kelly A. ; BenZvi, Segev

Abstract We explore how the definition of a void influences the conclusions drawn about the impact of the void environment on galactic properties using two void-finding algorithms in the Void Analysis Software Toolkit: Voronoi Voids ( V ² ), a Python implementation of ZOnes Bordering On Voidness ( ZOBOV ); and VoidFinder , an algorithm that grows and merges spherical void regions. Using the Sloan Digital Sky Survey Data Release 7, we find that galaxies found in VoidFinder voids tend to be bluer and fainter and to have higher (specific) star formation rates than galaxies in denser regions. Conversely, galaxies found in V ² voids show less significant differences when compared to galaxies in denser regions, less consistent with the large-scale environmental effects on galaxy properties expected from both simulations and previous observations. These results align with previous simulation results that show V ² -identified voids “leak” into the dense walls between voids because their boundaries extend up to the density maxima in the walls. As a result, when using ZOBOV -based void-finders, galaxies likely to be part of wall regions are instead classified as void galaxies, a misclassification that can be critical to our understanding of galaxy evolution.

• Sponsoring Organization: USDOE
• Grant/Contract Number: NONE; SC0008475
• OSTI ID: 2483618
• Journal Information: The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 978; ISSN 0004-637X
• Publisher: American Astronomical SocietyCopyright Statement
• Country of Publication: United States
• Language: English